Gl 63 Examination of DSS and 2MASS images shows two stars near the
Gl 63 GJ91 position at the epoch of the 2MASS images. GJ 63 is the
Gl 63 westernmost, high proper motion component of this optical
Gl 63 binary, and is 2MASS J01382162+5713571.
Gl 65 AB A=BL Cet, B=UV Cet
Gl 127.1 B Listed as an AB pair in the GJ91 catalog, with a separation of
Gl 127.1 B 8", but no position angle indicated. GJ 127.1 A is a
Gl 127.1 B well-known star with a Hipparcos position, so there is no
Gl 127.1 B difficulty identifying A. The Gliese catalog lists V=11.43,
Gl 127.1 B B-V=0.01 for A, V=14.73, B-V=0.62 for B. Caballero & Solano
Gl 127.1 B (2007ApJ...665L.151C), however, state that "The status of the
Gl 127.1 B hypothetical companion GJ 127.1 B is unknown". We examined all
Gl 127.1 B available online images of the field (including 2MASS, where
Gl 127.1 B the A-B contrast should be best) but found no sign of a B
Gl 127.1 B component, at any position angle, with a separation of 8"
Gl 127.1 B from A. We are therefore skeptical that B exists.
Gl 130 Examination of DSS and 2MASS finding charts shows a star of the
Gl 130 right magnitude, color, and proper motion within a few
Gl 130 arcseconds of the position indicated in the GJ91 catalog. This
Gl 130 star is 2MASS J03122972-3805204. We believe this is the
Gl 130 correct ID. This disagrees with the position listed in SIMBAD
Gl 130 (by about 30"), which is derived from Bakos
Gl 130 (2002, Cat. I/279). Our choice agrees with the position
Gl 130 reported by Rousseau & Perie (1997, Cat. J/A+AS/124/437).
Gl 293 Examination of the 2MASS and DSS finding charts shows a star of
Gl 293 the right proper motion at ~30" from the position indicated in
Gl 293 the GJ91 catalog. This star is 2MASS J07530814-6747314.
Gl 421 AB Gl 421 A and B form a visual binary separated on the sky by
Gl 421 AB about 20" (mostly east-west); Gl 421 C is ~4 mag fainter and
Gl 421 AB ~1.5' northwest from AB. The Hipparcos J2000, epoch 2000
Gl 421 AB coordinates for the AB pair are offset by nearly 5" from the
Gl 421 AB 2MASS epoch 2000 coordinates. Using the average of the
Gl 421 AB positions for Gl 421 C in UCAC3, HST-GSC2.3.2, and Lick NPM
Gl 421 AB (all agree to within 0.2") and measuring the offset from C to
Gl 421 AB A on DSS and 2MASS plates, we derive an epoch 2000 position
Gl 421 AB for A of 11 15 19.42, -18 08 40.2, which is nearly identical
Gl 421 AB to the 2MASS epoch 2000 position. We therefore adopt the 2MASS
Gl 421 AB positions for Gl 421 A and B. We also adopt our measured
Gl 421 AB proper motions for A and B (0.14"/yr in RA, -0.72"/yr in
Gl 421 AB DE), which agree well with the proper motion for C, but
Gl 421 AB disagree with the Hipparcos proper motion in RA (though this
Gl 421 AB does not explain the position offset between Hipparcos and
Gl 421 AB 2MASS).
Gl 451 B Discovered by van de Kamp in 1968 as an apparent flare star
Gl 451 B companion, separated by 2" from A. Not detected since 1968 to
Gl 451 B our knowledge (e.g., Heintz 1984PASP...96..557H).
Gl 452 B Identified as a faint, blue companion about 8" to east of
Gl 452 B Gl 452 A by Luyten. We see a star of the right magnitude and
Gl 452 B location in the 1954 blue DSS plate. However, it is not common
Gl 452 B proper motion with Gl 452 A. Reid & Gizis (2005, Cat.
Gl 452 B J/PASP/117/676) report they could not detect B at the expected
Gl 452 B position with the Keck I guide TV (at epoch ~2002), with an
Gl 452 B estimated limiting magnitude of R~21. We suspect Gl 452 B does
Gl 452 B not exist, at least as a physical companion to A.
Gl 534.1 B Location of B relative to A given incorrectly in GJ91. Correct
Gl 534.1 B relative position given in the Catalog of Components of Double
Gl 534.1 B and Multiple Stars (CCDM). Identification of B and
Gl 534.1 B confirmation of common proper motion with A made by
Gl 534.1 B examination of DSS and 2MASS finding charts.
Gl 549 C Gl 549 was listed as a triple system in Gl69, with the C
Gl 549 C component being located almost 1.5{deg} north of the AB pair.
Gl 549 C In GJ91, the C component was no longer listed as a member of
Gl 549 C the system. C is real, and does have a proper motion quite
Gl 549 C similar to the AB pair. However, its parallax is different
Gl 549 C from that of the AB pair (Gliese & Jahreiss,
Gl 549 C 1988Ap&SS.142...49G), and its spectral type and apparent
Gl 549 C magnitude are also inconsistent with forming a physical system
Gl 549 C with AB.
Gl 563.2 AB Alternate names for this binary are HIP 72509 and HIP 72511,
Gl 563.2 AB and Luyten Half-Second Catalogue (LHS) 379 and LHS 380.
Gl 563.2 AB Normally we would have just accepted the Hipparcos positions.
Gl 563.2 AB However, the J2000, epoch 2000 positions derived from the
Gl 563.2 AB Hipparcos data are clearly inconsistent with what is seen in
Gl 563.2 AB the DSS and 2MASS charts (see Fig. 1). The Hipparcos positions
Gl 563.2 AB indicate that the two stars are separated by 11" in RA and
Gl 563.2 AB 21.5" in DE. However, visual examination of the finding charts
Gl 563.2 AB clearly indicates the stars have separations more like 20"-25"
Gl 563.2 AB in RA and of order 10" in DE. We have chosen to adopt the
Gl 563.2 AB 2MASS positions for the system, and note that these positions
Gl 563.2 AB agree with what is given in the Hubble Space Telescope (HST)
Gl 563.2 AB GSC 2.2 and by the Carlsberg Meridian Catalog, while they
Gl 563.2 AB disagree by 10"-15" with the Hipparcos positions.
Gl 601 B The notes to G69 identify this star with L 153-157, with a
Gl 601 B position offset from the A component of 157" at position angle
Gl 601 B (PA) 258{deg}. A star with the expected motion is visible near
Gl 601 B the predicted position. The only astrometric catalog we can
Gl 601 B find for this star is the UCAC3, which lists
Gl 601 B 15 54 43.49, -63 26 14.8 (epoch 1998.3).
Gl 629.2 B The notes section of G69 indicates that this is a common proper
Gl 629.2 B motion companion to Gl 629.2 A. Giclas et al.
Gl 629.2 B (1960LowOB...4..136G) provide 1950 coordinates and a finding
Gl 629.2 B chart for Gl 629.2 B under the designation G17-27. That
Gl 629.2 B finding chart allows easy identification of this star as
Gl 629.2 B 2MASS J16352902-0357571.
Gl 732 B This star probably does not exist. Separation from A listed as
Gl 732 B about 10" and about 3.3mag fainter. Proper motion given as
Gl 732 B about 1.0"/yr to PA=161{deg}. Examination of the DSS and 2MASS
Gl 732 B charts shows no evidence for a companion to A. We could find
Gl 732 B no postdiscovery evidence in the literature that B exists.
Gl 734 AB The GJ91 catalog indicates that B is separated by 5.2" at
Gl 734 AB PA=21{deg} from A, with B being about 2.5 mag fainter than A
Gl 734 AB in the visual. Similar information is listed in the Washington
Gl 734 AB Double Star Catalog (WDS) and CCDM. Visual inspection of the
Gl 734 AB DSS and 2MASS images allows easy identification of A, but no
Gl 734 AB strong evidence for the presence of B. The 1952 DSS images
Gl 734 AB show a hint of extension in the north-south direction, with a
Gl 734 AB hint of a second set of diffraction spikes northward of the
Gl 734 AB main spikes, as expected. The 2MASS PSC shows two sources when
Gl 734 AB queried, the brighter being A and the fainter displaced from A
Gl 734 AB by about 4" to the north-northeast. This second source is
Gl 734 AB barely detected by 2MASS, but is at the approximate position
Gl 734 AB expected for B. We adopt the 2MASS coordinates; a better
Gl 734 AB measurement would be useful.
Gl 762 Nothing present within 30" of the GJ91 coordinate. Examination
Gl 762 of the DSS and 2MASS charts shows a star of the right
Gl 762 (relatively large) proper motion and colors about 45" from the
Gl 762 cataloged position. No other star of similar magnitude is
Gl 762 within 2.5'.
Gl 774 AB The Hipparcos input catalog lists GJ 774 A as an alias to
Gl 774 AB HIC 98811 A, providing a J2000 coordinate of
Gl 774 AB 20 04 02.1, -65 35 58.1. However, that is approximately the
Gl 774 AB correct coordinate for GJ 774 B (and about 20" from its true
Gl 774 AB position). HIP 98811 A should instead be aliased to GJ 774 B.
Gl 774 AB The GJ91 coordinate and proper motion allow the J2000 position
Gl 774 AB to be estimated to better than 30" accuracy, and the proper
Gl 774 AB motion is large enough to be distinctive, thus allowing easy
Gl 774 AB identification of the correct star.
Gl 781.1 AB The GJ91 catalog provides individual RA and DE values for both
Gl 781.1 AB components, with the secondary indicated as being 3 seconds
Gl 781.1 AB west and 18" north of the primary. When the GJ91 1950
Gl 781.1 AB coordinates are precessed, the proper motion corrected to
Gl 781.1 AB J2000, epoch 2000, and those positions checked versus the
Gl 781.1 AB 2MASS images, there are two relatively bright stars within a
Gl 781.1 AB few arcseconds of where they are predicted to be:
Gl 781.1 AB A, at 20 07 48.0, -31 45 30.0 (2000); and
Gl 781.1 AB B, at 20 07 45.0, -31 45 14. (2000). Comparing the 2MASS and
Gl 781.1 AB DSS images shows those stars to both have the proper motions
Gl 781.1 AB expected (0.8"/yr toward PA 159{deg}). The only problem is
Gl 781.1 AB that Gl 781.1 A was included in the Hipparcos input catalog as
Gl 781.1 AB HIC 99150. A star was found by Hipparcos at almost exactly the
Gl 781.1 AB predicted HIC location, and subsequently HIP 99150 was given
Gl 781.1 AB the Hipparcos 1997 position of 20 07 44.98, -31 45 14.4 (2000)
Gl 781.1 AB Unfortunately, based on the data in GJ91, this star is not
Gl 781.1 AB Gl 781.1 A but is instead Gl 781.1 B. SIMBAD adopted the
Gl 781.1 AB Hipparcos identification, and called the star at
Gl 781.1 AB 20 07 48.0, -31 45 30 Gl 781.1 B. We prefer to retain the
Gl 781.1 AB positional reference data from the GJ catalog itself, making
Gl 781.1 AB the A component the southeastern star of the binary. The two
Gl 781.1 AB stars have very similar luminosities.
Gl 806.1 B The A component of this system is a V=2.45, K giant. According
Gl 806.1 B to GJ91, the B component is located 6 seconds west and 6"
Gl 806.1 B south from A, and is listed as a V=13.4, M4 dwarf. We could
Gl 806.1 B not confirm B by its proper motion using the DSS and 2MASS
Gl 806.1 B charts because the image of A is so bright. However, the 2MASS
Gl 806.1 B images show two stars at about the expected position for B.
Gl 806.1 B Neither star is in the online 2MASS PSC. However, both stars
Gl 806.1 B are in the 2MASS "working database". One of this pair is too
Gl 806.1 B blue to be an M star. The brighter and more northwest of this
Gl 806.1 B pair does have near-IR colors compatible with being an M4
Gl 806.1 B dwarf. That star is at 20 46 06.39 +33 58 06.1 (2000),
Gl 806.1 B observed by 2MASS on 1999 May 16, with J=9.456, H=8.889,
Gl 806.1 B K=8.649 (uncertainties of 0.031, 0.015, and 0.009; data from
Gl 806.1 B the 2MASS working database).
Gl 871.1 AB This binary appears in the Gl69 catalog, but not in GJ91.
Gl 871.1 AB Spectral types are listed as M3 and M4. The positions in Gl69
Gl 871.1 AB were only given to a precision of 0.1 minute of time, and 1'
Gl 871.1 AB of declination; the pair has negligible proper motion. No star
Gl 871.1 AB appears within 1' of the stated position on the DSS and 2MASS
Gl 871.1 AB charts, but the binary is clearly identifiable on those charts
Gl 871.1 AB (based on relative position and colors) about 2' west of the
Gl 871.1 AB cataloged position.
GJ 1001 AB GJ 1001 was listed as a single star in the GJ79 update to the
GJ 1001 AB Gliese catalog. Using the coordinates from GJ79, no compatible
GJ 1001 AB object is within 1' on the DSS or 2MASS charts. However, a
GJ 1001 AB star with the right proper motion (1.6"/yr toward PA=155{deg})
GJ 1001 AB is visible about 2' south of the expected position. A common
GJ 1001 AB proper motion companion is also visible in those charts to the
GJ 1001 AB west of the primary. This pair is now referenced as GJ 1001 A
GJ 1001 AB and 1001 B (see Goldman et al. 1999A&A...351L...5G).
GJ 1001 AB Both stars have 2MASS counterparts, which we have adopted for
GJ 1001 AB our position reference.
GJ 1022 Examination of DSS and 2MASS charts showed no star within 1' of
GJ 1022 the expected position from GJ91. However, a star matching the
GJ 1022 cataloged proper motion (1.119"/yr to PA=94{deg}) is easily
GJ 1022 identifiable on those charts about 1.5' from the GJ91
GJ 1022 position. The 2MASS colors of that star
GJ 1022 (2MASS J00492903-6102326) are compatible with the late-M
GJ 1022 spectral type given for this star by GJ91.
GJ 1167 B GJ 1167 A is easily identified in DSS and 2MASS charts, within
GJ 1167 B 15" of the position given by GJ91. GJ91 states that "comp B
GJ 1167 B doesn't exist". However, in the GJ79, a GJ 1167 B is listed
GJ 1167 B (at a position about 80" east and 3' north of the A position).
GJ 1167 B A star is present in the DSS and 2MASS charts within about 15"
GJ 1167 B of the GJ79 prediction, and with proper motion between the
GJ 1167 B 1955 epoch DSS and 2000 epoch 2MASS charts essentially
GJ 1167 B identical (to the eye) to the A component. The photometry for
GJ 1167 B B is significantly bluer than for A, however, which seems
GJ 1167 B unphysical since A is 2-4 mag brighter than B. This suggests
GJ 1167 B the pair is not a physical binary, in agreement with the
GJ 1167 B statement in GJ91.
GJ 1287 Despite a true position more than 30" from what is given in
GJ 1287 GJ79, this star is easily identified on DSS and 2MASS charts
GJ 1287 due to its large proper motion (0.9"/yr to PA=98{deg}). It was
GJ 1287 not included in GJ91 because newer distance estimates place it
GJ 1287 beyond 25 pc.
GJ 2013 Examination of DSS charts shows no good candidate within 1' of
GJ 2013 the GJ79 position. We identified the star using the finding
GJ 2013 chart in Eggen (1968ApJ...153..723E). This star is not
GJ 2013 included in GJ91 because the revised distance estimate places
GJ 2013 it beyond 25 pc.
GJ 2014 An accurate position for this star is provided by Costa et al.
GJ 2014 (2006AJ....132.1234C). The corresponding 2MASS object is
GJ 2014 2MASS J00495863-2624055. The near-IR and V-K colors agree with
GJ 2014 that expected for the B-V color listed in GJ79. This star was
GJ 2014 not included in GJ91.
GJ 2023 This is a very faint star with quite small proper motion. It is
GJ 2023 therefore not possible to identify it unambiguously using the
GJ 2023 DSS and 2MASS charts. Friedrich et al. (2000,
GJ 2023 Cat. J/A+A/363/1040) were able to identify it and obtained
GJ 2023 spectra confirming it as a white dwarf. Using the coordinates
GJ 2023 provided in that article, we identify GJ 2023 as
GJ 2023 2MASS J01295612-3055098.
GJ 2052 This is a faint, bluish star with little proper motion. Only
GJ 2052 one star is present within 30" of the predicted position on
GJ 2052 the DSS charts. That star is not present in the 2MASS PSC,
GJ 2052 because it is too faint. A blue star with nearly the same V
GJ 2052 magnitude as listed in GJ79 and located within 5" of the GJ79
GJ 2052 position is present in the Lick Northern Proper Motion Survey
GJ 2052 (Klemola et al. 1987, Cat. I/199). We adopt their position.
GJ 2087 There is no star in the DSS or 2MASS charts at the J2000 GJ91
GJ 2087 position and Bakos et al. (2002, Cat. I/279) claim this is a
GJ 2087 plate flaw.
GJ 2133 This star is located in a very crowded field. No object with
GJ 2133 the expected proper motion and color is present on the DSS and
GJ 2133 2MASS charts within 1' of the cataloged position. A star with
GJ 2133 the expected characteristics is present on those charts about
GJ 2133 1' west and 30" south of the cataloged position. That star
GJ 2133 is 2MASS J17540302-3440177.
GJ 2154 AB Examination of the DSS charts showed no stars matching the
GJ 2154 AB expected properties within 1' of the cataloged position.
GJ 2154 AB However, the binary is easily identifiable about 1.5' away,
GJ 2154 AB based on the relatively large proper motion and the
GJ 2154 AB appropriate separation and position angle.
GJ 3063 This should be a relatively bright (V=11.9) M3 star of low
GJ 3063 proper motion according to the GJ91 catalog. However, only two
GJ 3063 stars appear in the 2MASS images near the cataloged position,
GJ 3063 and neither are particularly red. No star of approximately the
GJ 3063 right properties is present in, for example, the USNO B1 or
GJ 3063 HST GSC within several arcminutes of the expected position.
GJ 3063 The only alias in GJ91 is to Sm177 (Smethells 1974, Ph.D.
GJ 3063 thesis, Case Western Reserve Univ.), and SIMBAD provides no
GJ 3063 literature references. We were unable to recover this star.
GJ 3085 No star of the expected properties is located on the DSS charts
GJ 3085 within 1' of the position listed in GJ91. A finding chart is
GJ 3085 provided in Pesch & Sanduleak (1978AJ.....83.1090P); based on
GJ 3085 that chart, we identify GJ 3085 as being located about 2.2'
GJ 3085 north and 1' east of the cataloged position. Its near-IR
GJ 3085 colors are consistent with the "m" spectral type provided
GJ 3085 in GJ91.
GJ 3096 No star of the expected properties is located on the DSS charts
GJ 3096 within 1' of the position listed in GJ91. A finding chart is
GJ 3096 provided in Pesch & Sanduleak (1978AJ.....83.1090P); based on
GJ 3096 that chart, we identify GJ 3096 as being located about 1.2'
GJ 3096 north and 0.4' west of the cataloged position. Its near-IR
GJ 3096 colors are consistent with the "m" spectral type provided
GJ 3096 in GJ91.
GJ 3101 No star of the expected properties is located on the DSS charts
GJ 3101 within 1' of the position listed in GJ91. Reid et al. (1995,
GJ 3101 Cat. III/198) list a position for GJ 3101 that is more than 5'
GJ 3101 different from that in GJ91. Comparison of the DSS chart at
GJ 3101 the Reid et al. position to a finding chart in Pesch &
GJ 3101 Sanduleak (1978AJ.....83.1090P) allows identification of
GJ 3101 GJ 3101 (aka PS244). This star is 2MASS J01360872-2652161; the
GJ 3101 near-IR colors are consistent with the "m" spectral type
GJ 3101 listed in GJ91.
GJ 3397 Inspection of the DSS images shows a star with the correct
GJ 3397 colors and proper motions about 0.8' south and 0.1' east of
GJ 3397 the coordinates in the GJ91 catalog. This star is
GJ 3397 2MASS J06322189-6957445.
GJ 3521 Examination of the DSS charts shows no appropriate star at the
GJ 3521 cataloged position. A star with the expected proper motion,
GJ 3521 magnitude, and colors is present about 1' west and 10" south
GJ 3521 of the GJ91 position. This star is 2MASS J08550473-7135480.
GJ 3592 We used the finding chart provided by Eggen
GJ 3592 (1969ApJ...157..287E) to identify this star on the 2MASS
GJ 3592 charts. This object is 2MASS J10145842-5611114. This position
GJ 3592 agrees with that given by Wegner (1973MNRAS.163..381W).
GJ 3618 The very large proper motion of this star (1.5"/yr) makes its
GJ 3618 identification on DSS and 2MASS charts easy despite the more
GJ 3618 than 1' error in the cataloged position.
GJ 3999 A/4000 B This is a binary separated by ~30" at PA=338{deg}.
GJ 3999 A/4000 B Identification is made difficult because GJ 3999 A is passing
GJ 3999 A/4000 B very near a much brighter field star at 2MASS epoch (see
GJ 3999 A/4000 B Fig. 1). Its distinctive proper motion and colors make the
GJ 3999 A/4000 B identification secure.
GJ 4012 No star evident on the DSS and 2MASS charts within 2' of the
GJ 4012 cataloged position. We used a finding chart from Luyten
GJ 4012 (1949ApJ...109..528L), under the alias L270-37, to identify
GJ 4012 the star on the DSS charts, and to confirm its proper motion
GJ 4012 by comparison to 2MASS charts. Our 2MASS-based J2000 position
GJ 4012 is within ~5" of the position listed by Downes et al.
GJ 4012 (2001, Cat. V/123).
GJ 4028 Cataloged position in error by ~1.5'. High proper motion
GJ 4028 makes identification on DSS and 2MASS charts secure.
GJ 4078 There is a star 2.2' east and 1' south of the GJ91 coordinate
GJ 4078 in the DSS images, whose colors and proper motion match those
GJ 4078 expected for GJ 4078. This star is 2MASS J18495119-5726486.
GJ 4078 SIMBAD lists the star at this position as LHS 3413, one of the
GJ 4078 aliases given for GJ 4078 in the GJ91 catalog.
GJ 4088 In the GJ91 catalog, GJ 4088 is aliased to LP 571-80. LP 571-80
GJ 4088 is aliased to HIC 93047 in the HIC. However, the position
GJ 4088 given in the HIC is considerably in error, and presumably as
GJ 4088 a result no useful data were obtained by Hipparcos for this
GJ 4088 star. The coordinates given in the GJ91 catalog are in error
GJ 4088 by less than 30", allowing easy identification of the correct
GJ 4088 star based on its proper motion and magnitude.
GJ 4103 Very little information for this star is given in GJ91. An
GJ 4103 alias is given to LP 336-6 (ver. 1 of the New Luyten
GJ 4103 Two-Tenths Catalogue [NLTT]), and the listed position and
GJ 4103 proper motion are taken directly from the NLTT (or from the
GJ 4103 Bruce Proper Motion Survey [BPM] catalog, where it is listed
GJ 4103 as BPM94000). However, no object with the listed proper motion
GJ 4103 is present within 2.5' of the listed position. A star of
GJ 4103 somewhat similar position and proper motion is present several
GJ 4103 arcminutes north of the listed position, but that star is
GJ 4103 identified in the NLTT as LP 336-7, and we do not believe
GJ 4103 there is enough information to equate that star to GJ 4103. We
GJ 4103 do note that there is a third NLTT star somewhat nearby in
GJ 4103 space whose listed red and blue magnitudes and proper motion
GJ 4103 size and direction are exactly equal to those for LP 336-6;
GJ 4103 this other object is LP 336-2. A barely resolved binary of the
GJ 4103 appropriate general brightness and proper motion is present on
GJ 4103 the DSS and 2MASS charts at about the position listed for
GJ 4103 LP 336-2; this pair is 2MASS J19050788+3237547 and
GJ 4103 2MASS J19050756+3237526. Weis (1987AJ.....93..451W) also noted
GJ 4103 the exact duplication of information in the NLTT for these two
GJ 4103 LP stars, and that no obvious candidate was present at the
GJ 4103 listed position for LP 336-6. Our conclusion (similar to
GJ 4103 Weis), is that either LP 366-6 does not exist, or it is
GJ 4103 probably the same object as LP 336-2.
GJ 4112 The DSS images show a bright star 30" east and 8" north of the
GJ 4112 GJ91 coordinates whose proper motion and colors match those
GJ 4112 expected for GJ 4112. This star is 2MASS J19340394-5225144.
GJ 4112 Pokorny et al. (2004, Cat. J/A+A/421/763) list the star at
GJ 4112 this position as having a proper motion consistent with that
GJ 4112 given in the GJ91 catalog, and indicate this star is L275-26,
GJ 4112 one of the aliases listed in the GJ91 catalog for GJ 4112.
GJ 4133 High proper motion star (1.08"/yr). The DSS images have a
GJ 4133 bright star 1.1' east and 45" south of the GJ coordinates
GJ 4133 whose proper motion and colors match those expected for
GJ 4133 GJ 4133. This star is 2MASS J20053482-1056545. SIMBAD matches
GJ 4133 this star to LHS 483 and LP 754-16, both aliases for GJ 4133
GJ 4133 given in the GJ91 catalog.
GJ 4187 A/4188 B True position slightly more than 30" different from GJ91
GJ 4187 A/4188 B coordinates, but binary easily identifiable on DSS and
GJ 4187 A/4188 B 2MASS charts.
GJ 4189 A/4190 B These two binary components have a separation of 4" in the GJ91
GJ 4189 A/4190 B catalog and a PA of 341{deg} in the WDS catalog. The stars are
GJ 4189 A/4190 B of a similar spectral type and are resolved in the DSS images
GJ 4189 A/4190 B where it is clear they share a common proper motion. Using the
GJ 4189 A/4190 B information in the WDS catalog we conclude that GJ 4190 B is
GJ 4189 A/4190 B the more northerly star. This disagrees with the GJ91
GJ 4189 A/4190 B information (which traces back to the NLTT), but agrees with
GJ 4189 A/4190 B the double star measures of Worley (1962AJ.....67..403W).
GJ 4191 The GJ91 catalog indicates this star is a white dwarf with a
GJ 4191 relatively high proper motion. Examination of DSS images shows
GJ 4191 a blue star 90" east and 15" north of the GJ position that has
GJ 4191 about the right proper motion. That star is
GJ 4191 2MASS J21193652-5550144.
GJ 4193 DSS and 2MASS charts show no appropriate match within 1' of
GJ 4193 the input coordinate. There is a star of the right magnitude
GJ 4193 and color about 20" east and 1.6' south of the GJ coordinate.
GJ 4193 This star is 2MASS J21261422-4227320. Hawley et al.
GJ 4193 (1996, Cat. III/198) give this as the coordinate for
GJ 4193 BPM 43997, which is one of the aliases listed for GJ 4193 by
GJ 4193 the GJ91 catalog.
GJ 4224 AB No star is visible in the DSS or 2MASS charts within 1' of the
GJ 4224 AB expected position based on GJ91 1950 position and proper
GJ 4224 AB motion. A star with the right magnitude, colors, and proper
GJ 4224 AB motion (0.34"/yr to PA=121{deg}) is present about 1' east and
GJ 4224 AB 1.5' south of the GJ91 position. The GJ91 catalog does not
GJ 4224 AB provide PA or separation, but reports a difference in
GJ 4224 AB magnitude of 0. On the DSS charts, the star we have identified
GJ 4224 AB as GJ 4224 has faintly visible double diffraction spikes,
GJ 4224 AB indicating a binary separated approximately north-south by a
GJ 4224 AB few arcseconds. Weistrop (1980AJ.....85..738W) states that
GJ 4224 AB GJ 4224 (under the alias Sm 89) "appears double at the
GJ 4224 AB telescope", also indicating the separation is probably on the
GJ 4224 AB order of 2"-3". Based on its J2000 coordinate, the star we
GJ 4224 AB have identified as GJ 4224 is also HIP 107711. We use the
GJ 4224 AB Hipparcos position for both components.
GJ 4237 A/4238 B Listed in the GJ91 catalog as being separated by 3.4", but no
GJ 4237 A/4238 B PA given. The 2MASS catalog lists two stars of about the right
GJ 4237 A/4238 B magnitude and separation very near the GJ91 input position.
GJ 4237 A/4238 B These two stars are 2MASS J21553860+3302138 and
GJ 4237 A/4238 B 2MASS J21553870+3302106. The WDS indicates that B is south
GJ 4237 A/4238 B of A, therefore we match GJ 4237 A to 2MASS J21553860+3302138,
GJ 4237 A/4238 B and GJ 4238 B to 2MASS J21553870+3302106.
GJ 4249 There is no star of appropriate magnitude within 2' of the GJ91
GJ 4249 position. A bright star with the appropriate (large) proper
GJ 4249 motion is, however, easily found on the DSS and 2MASS charts
GJ 4249 about 3' east of the cataloged position. Based on the J2000
GJ 4249 position and magnitude, this star is HIP 108890. We adopt
GJ 4249 the Hipparcos position for GJ 4249.
GJ 4327 There are two stars with essentially equal brightness at the
GJ 4327 position indicated by GJ91. The westernmost of the pair is
GJ 4327 redder and has high proper motion to the south, as expected;
GJ 4327 we identify this star as GJ 4327. It is
GJ 4327 2MASS J23172441+3812419. GJ91 lists LHS 3293 as an alias.
GJ 4327 Unfortunately, the HIC aliases LHS 3293 to HIP 114994, the
GJ 4327 easternmost (approximately stationary) star of the pair. We
GJ 4327 disagree with this latter alias, and instead alias LHS 3293 to
GJ 4327 the 2MASS star indicated above.
GJ 4386 There is no appropriate star within 30" of the GJ91
GJ 4386 coordinates; however, a star of the right magnitude, color,
GJ 4386 and proper motion (based on examination of DSS and 2MASS
GJ 4386 finding charts) is present abut 60" south and 15" west of
GJ 4386 the original coordinate. This star is 2MASS J23594483-4404599.
GJ 4386 SIMBAD cross-identifies this star with LTT 9828 and
GJ 4386 LP 988-175, both aliases for GJ 4386 listed in GJ91. The J-K
GJ 4386 color for this star seems much too blue for the M7 spectral
GJ 4386 type listed in GJ91. The actual spectral type is probably much
GJ 4386 earlier; Reid et al. (1995, Cat. III/198) give the spectral
GJ 4386 type as M2.
Wo 9354 The Wo70 catalog indicates that this star is Vyss 606
Wo 9354 (Vyssotsky 1956, Cat. III/13). There is no star that matches
Wo 9354 the expected properties within 1' of the input position. Only
Wo 9354 one star of about the right magnitude and color is present
Wo 9354 within about 2.5' of the Woolley coordinate; it is
Wo 9354 2MASS J11163293+2627415. Examination of the HIC indicates that
Wo 9354 this star is HIP 55077; the HIC provides a
Wo 9354 cross-identification to Vyss 606, confirming the
Wo 9354 identification.
Wo 9358 No star of the appropriate properties falls within 1' of the
Wo 9358 Woolley catalog position. A star of the correct (but
Wo 9358 relatively small) proper motion and with the correct
Wo 9358 approximate magnitude lies about 3' south of the Woolley
Wo 9358 position. This star is also HIP 55605.
Wo 9540 C The A component of this system is V=4.2. According to GJ91, the
Wo 9540 C C component is separated from A by 7.6" at PA=53{deg}. C is
Wo 9540 C not present in the 2MASS PSC. Because A and B are so bright, C
Wo 9540 C cannot be identified on the DSS or 2MASS charts. However, a
Wo 9540 C star in the right position relative to A is present in the
Wo 9540 C HST GSC2.3.2, and we adopt the coordinate from that source
Wo 9540 C for Wo 9540 C.
Wo 9785 This star is the exciting source for the planetary nebula
Wo 9785 NGC 7293. Use of IRSA's FINDER allows relatively secure
Wo 9785 identification of the star and a match to
Wo 9785 2MASS J22293854-2050136.
Wo 9805 No star of the appropriate properties falls within 2' of the
Wo 9805 Woolley catalog position. However, the Woolley catalog
Wo 9805 indicates that Wo 9805 is also Vyss 856, and the HIC
Wo 9805 cross-matches Vyss 856 to HIP 113782. We confirm that the
Wo 9805 colors and (small) proper motion of the star at the Hipparcos
Wo 9805 position agree with expectations for Wo 9805 given its
Wo 9805 spectral type of M0.5 and BVRI photometry provided in
Wo 9805 Laing (1989SAAOC..13...29L).